Primordial non-Gaussianity from the large-scale structure

By V. Desjacques, Uros Seljak. 2010

149 citations recorded by the source corpus.

Primordial non-Gaussianity is a potentially powerful discriminant of the physical mechanisms that generate the cosmological fluctuations observed today. Any detection of non-Gaussianity would have profound implications for our understanding of cosmic structure formation. In this paper, we review past and current efforts in the search for primordial non-Gaussianity in the large-scale structure of the Universe.

Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/bfd26d987e8b722ab94a960bf6065c21975cb41f

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In Astronomy and Astrophysics

  1. Daniel J. Eisenstein
  2. Uros Seljak
  3. F. Beutler
  4. C. Porciani
  5. A. Pillepich
  6. Tommaso Giannantonio
  7. Adam Amara
  8. J. Carron

In Statistical and Nonlinear Physics

  1. Uros Seljak
  2. Daniel J. Eisenstein
  3. F. Beutler
  4. Yu Feng
  5. Zachary Slepian
  6. Adam Amara
  7. Yin Li
  8. Tommaso Giannantonio

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